The DV bootstrap result for Kepler-186f in the Q1–Q17 DR25 transit search is shown in Fig. REF . Kepler-186f is a confirmed Terrestrial-sized planet orbiting in or near the HZ of a cool M-dwarf [1]}. The false alarm probability curve as determined from the null event statistics for trial pulse duration \(= 5\)  hr is plotted as a function of detection statistic. Given MES \(= 7.7\sigma \)  for Kepler-186f, the probability of false alarm was estimated to be 2.97x\(10^{-13}\) . This is equivalent to a \(7.2\sigma \)  detection on a Gaussian distribution. The detection threshold on the MES distribution derived from the null statistics in this case would have to be \(7.6\sigma \)  in order to achieve the same false alarm probability as a \(7.1\sigma \)  threshold on a Gaussian distribution.
<FIGURE>